Detector | Exposure (Original/Cleaned) | Image binning | Plate scale ("/pixel) | Bgd. level (orig/cleaned, counts/sq. arcmin/s) | GTI file | Bgd. light curves | Roll angle | CCD counts | Extra info |
---|---|---|---|---|---|---|---|---|---|
ccd6 | 14918 | 14918 | 1.00 | 0.49 | 0.0031/0.0031 | Yes | orig clean | |||
ccd7 | 14918 | 14918 | 1.00 | 0.49 | 0.0065/0.0065 | Yes | orig clean | |||
acis | 14918 | 14918 | 4.00 | 1.97 | 0/0 | Yes | orig clean | ccd6:3433 ccd7:7225 ccd8:3034 |
datamode=VFAINT readmode=TIMED gainfile=acisD2000-01-29gain_ctiN0006.fits CCD Temp=-120 object=PSR J1846+0919 firstrow=1 ACIS data processing version=8.4.5 nrows=1024 date-obs=2012-06-12T07:17:44 roll_angle=148.335409973 Original CALDB version=4.4.10 timedel=3.14 (full readout) CIAO_version=CIAO 4.3 |
25 source(s) in memory Iteration: 2 Images: |ccd6 |ccd7 |acis |
|
|
Python version = 2.5.4 (r254:67916, Aug 14 2009, 18:07:15) [GCC 4.1.1 20070105 (Red Hat 4.1.1-52)]
Headas version = 6.11
CIAO version = 4.3.0
XAssist version = 1.000
numpy version = 1.3.0
Pyfits version = 2.1.1
XAssist originally started on this data set at Wed Jun 26 13:49:03 2013
This data set was last accessed on Wed Jun 26 13:49:03 2013
Current user = xassist on xassist.localdomain
Number of fields in memory = 1
Current field being processed = acisf13793
Position of field target = 18 46 26.00 9 19 46.0
Current telescope = chandra
Current detector = acis
Processing mode = proc
Processing status = OK
Detection method = wavelet
Batch processing enabled
Place data, logs, etc. in field subdirectories
Image analysis will be over range of allowed energies
Will analyze each ccd separately
Will skip analysis of CCD 8
Log files: processing messages |error messages |all messages (very detailed) |source logs